Can We Measure the Higgs Boson's Quantum Numbers?

Total Page:16

File Type:pdf, Size:1020Kb

Can We Measure the Higgs Boson's Quantum Numbers? Can we measure the Higgs boson’s quantum numbers? D.J. Miller University of Glasgow 22 nd November 2007 Outline: Introduction The Higgs boson’s Spin The Higgs boson’s CP CP Violating Higgs bosons Conclusions Are secrets of the universe just about to be revealed? The invisible force which explains the nature of life, the universe and everything was first predicted by an Edinburgh scientist. Now, a team of Glasgow University physicists are preparing to discover if he was right. "The exciting thing is that we have no idea what we will find," say Parkes. " It could be the Higgs boson, or it could be something else entirely.” At dinner parties, Dr Parkes is often too embarrassed to admit what he does for a living. There is even a plucky band of space boffins … [led] by an English ex-pop star. You couldn’t make it up. Physicist Brian Cox, an expert on the forces created by the Big Bang and science adviser on Sunshine, played keyboards for Nineties rock group D:Ream. Almost right! (missed gW) This is just a tiny part of an equation which stretches to 36 lines. Scientists say it explains everything in the universe. The only trouble is that one of its key ingredients, the Higgs particle represented by the letter H, has never been found. CERN hope their particle machine will find the missing clue. Brian says: “It explains everything in physics from why is the sky blue to why chemistry works.” They are just one of the things Brian and his colleagues hope to find in a £2BILLION project to blast, pulverise and smash the atom in a recreation of the forces unleashed by the Big Bang…. 1. Introduction (or Tevatron) If the Higgs boson exists, it is almost certain that the LHC will see it within 10fb -1 or so: Notice that heavier Higgs bosons are dominated by leptons. I have a question for the experimenters about CMS’s figures (I know this is the wrong audience….) CMS Also produce a “required luminosity” plot: How can we reconcile these plots? This reflects the Higgs decay branching ratios: For low Higgs mass, the Higgs predominantly decays to b-quarks For higher Higgs mass, the Higgs predominantly decays to gauge bosons. The leptons is more significant than because it is so clean. We have good indications that the Higgs boson will be reasonably light: triviality vacuum stability Electroweak precision data: (95% conf.) Folding in LEP limit gives (95% conf.) [Numbers from Terry Wyatt’s talk at EPS 07] Imagine we discover a “Higgs-like” resonance at the LHC. How do we know that it is the Higgs boson? We need to measure: Higgs CP and spin The Higgs is a pretty weird object – we have never seen a fundamental scalar before. Also should ensure it is not a pseudoscalar, or a mixture of scalar and pseudoscalar. Higgs couplings to fermions and gauge bosons Must be proportional to the particle masses Higgs self couplings In principle allows us to reconstruct the Higgs potential (out of reach of the LHC) The first 2 are intimately linked since CP and spin restrict the form of the couplings. In this talk, I will concentrate on the first requirement: Higgs CP and spin I consider a reasonably heavy Higgs boson, 150 - 200 GeV, and look at its decay All the information on the Higgs spin Z and CP is contained in this vertex H Z Our approach: Write down the most general vertex for a particle of a particular spin and CP coupling to ZZ and see how it differs from the SM Higgs. In principle, there are lot of other production mechanisms, decays and couplings one could exploit. For example, Production at LHC: (W boson fusion) Production at ILC: Decays: [see arXiv:0708.0458 for references] 2. Higgs boson spin (or lack thereof) Let’s start with an example: distinguishing the SM state from an axial vector SM coupling: General axial-vector coupling: “constants” could be Z momenta: (dimensionless) functions of momenta Notice that the 0 - terms always contain a momentum dependence, unlike the SM. Examine the dependence of the cross-section on the virtuality of the off-shell Z boson: β is the Z*/Z three-momentum in the H rest frame, in units of the Higgs mass M H. This β comes from phase space , not the Higgs properties. ⇒ At threshold ( β → 0) dependence on β is linear. By contrast, for the axial-vector, the cross-section is [helicity amplitudes] ⇒ At threshold ( β → 0) have β3 rise. This is reflected for almost all spin choices: normality For even normality, only spin 0 and spin 2 give ΓH ∼ β O(1) is caused by gµ β1 gν β2 term in coupling. (I will come back to this.) For odd normality, only spin 1 shows Γ ∼ β The time only 1 + has a linear dependence. Higher spins ( ≥ 3) always show a steeper dependence on β Even normality: Odd normality: So, an observation of a β dependence near threshold rules allows only 0 +, 1 - or 2 + If we set the dangerous terms to zero , and (Even normality only) dependence dependence dependence Ruling out the dangerous terms: If we see or then 1 - (in fact any odd spin) is ruled out generally by Yang’s theorem Alternatively use angular correlations of the leptons SM has By contrast 0 - has so no term And the offending spin-2 term causes all so contains terms such as which are absent in the SM. 3. CP Quantum Numbers You may have noticed in the above that we also had 0 -, so we can use the same ideas to check the CP of the Higgs. A CP odd term must take the form which leads to SM here included ΓZ for both Z’s CP odd Alternatively (or above the ZZ threshold), one can use angular distributions again. This provides a very clear distinction between 0 + and 0 - states. Standard Model CP odd 4. CP violating Higgs couplings The most general vertex for a spinless particle coupling to a Z boson is SM coupling (CP even) CP even CP odd The SM is given by a=1, b=c=0. a can always be chosen to be real, but b and c can be complex. Note that and simultaneously CP violation But or CP is conserved since it may just be that the Z couples to the CP even or CP odd part A note on gauge invariance This vertex manifestly doesn’t satisfy the expected Ward identities: i.e . and In principle, one could make the extra terms in the vertex satisfy these identities by rewriting them as, for example Notice that this term still breaks the Ward identities, but this is not surprising since the Ward identities are broken also for the SM. This is because electroweak symmetry is already broken. The Ward identities only need to hold in the limit The above vertex is equivalent to the original vertex with a redefinition of a and b since extra terms like will vanish when contracted with conserved currents. The total rate The most obvious expectation is to have a SM like coupling plus an extra CP violating part, i.e and c small This will boost (or shrink) the total rate for Can we distinguish the extra couplings via that total width to Z’s? m m 1 and 2 are the virtualities of the Z-bosons, which must be integrated over Examine the total number of events observed in leptons as according to the ATLAS TDR study [Hohlfeld, ATL-PHYS-2001-004] . Initial cuts: Two leptons with Two additional leptons with All four leptons with rapidity Compare signal with background in a small window around mH and usual lepton identification and reconstruction efficiency applied. Additionally: For mH = 150 GeV, + impact parameter and isolation cuts For mH = 200 GeV, + pT of hardest Z Notice that there were no K factors in the ATLAS study. For the production this may enhance the rate by up to a factor 2 For the decay, NLO changes the rate by about 5% The ATLAS study found: For and signal: 67.6 events background: 8.92 events For and signal: 54 events background: 7 events The number of signal events will be increased or decreased by our altered coupling, but the backgrounds will stay the same. We assumed that the effect of the cuts on the signal is the same as the SM. We only allowed the HZZ coupling to change. In principle, the same physics that changes the HZZ coupling may change the HWW coupling. Although this wouldn’t effect the HZZ width, it would effect the HZZ branching ratio. Set b=0 for simplicity Scale up to SM NS is the number of signal events in the SM, and we calculated the number with an altered coupling N S. If the number of background events is N B, then we expect a typical fluctuation of the SM total events to be Then the significance of any deviation is Deviation from the SM (with b=0) 3-5 >5 σ σ <3 σ It is impossible to tell whether the difference arises from an overall factor (e.g. bigger a) or a new term in the coupling. So the total rate is not a lot of use. Also, we can’t measure the phase of c. Threshold behaviour Previously we saw how the threshold behaviour could distinguish a CP even and CP odd state. Can we do the same with a CP-violating vertex? Only one term (the square of the CP-even part) has a linear dependence on β (this comes from the phase space) However, this term will dominate the threshold dependence as long as .
Recommended publications
  • Prof. Terry Wyatt FRS Employment History Education Fellowships And
    CURRICULUM VITAE — Prof. Terry Wyatt FRS Born: 29th June 1957, Watford, England. Nationality: British. Family Status: Married, with two sons. Employment History Tenured Physics Faculty: School of Physics and Astronomy, University of Manchester, UK. – Professor (2004–present) [DØ and ATLAS experiments] – Reader (1999–2004) [OPAL and DØ experiments] – Lecturer (1996–1999) [OPAL experiment] – Senior visiting appointments, on leave from usual academic duties at University of Manchester: Guest Scientist, Fermilab: 15 month period as Paid Guest Scientist at Fermilab (2002–2003) PPARC Senior Research Fellowship: 3-year period (2003-2006) STFC support for DØ spokesperson: 100% salary buy-out for 18 month period (2006–2007). As spokesperson of DØ I also received financial support from Fermilab. – I currently serve as Chair of the Accelerator, Nuclear and Particle Physics Division of the School of Physics and Astronomy, with overall responsibility for both experimental and theoretical aspects of these fields. PPARC Advanced Research Fellow: Based at CERN with University of Manchester, UK. (1989–1996). [OPAL experiment]. PPARC Research Associate: QMC, University of London, UK. (1986–1989). [OPAL experiment] CERN Fellow: CERN, Geneva, Switzerland. (1984–1986). [UA1 experiment] Education Research Student: University of Oxford, UK. (1979–1983). [TASSO experiment] Degree: D.Phil. Undergraduate Student in Physics: Imperial College, University of London, UK. (1976–1979). Degree: B.Sc. (Ist class hons. Awarded governors’ prize for top first in physics, 1979). Associateship of the Royal College of Science (A.R.C.S). Fellowships and Prizes • Elected as Fellow of the Royal Society, FRS (2013). Excerpt from citation: “Distinguished for a number of original and important contributions to the experimental verification of the Standard Model”.
    [Show full text]
  • Sandbox Studio 9 Symme
    it on symmetry | volume 03 issue 10 december 06 Photos: Sandbox Studio 9 Physicist Michael Weber (right, Fermilab) and his colleagues (from left) Michael Kirby (Radboud University Nijmegen, Netherlands), Chris Neu (University of Pennsylvania), Sabine Lammers (Columbia University), Ben Kilminster (Ohio State University) as well as other experimenters at CDF and DZero are hitting upon numerous discoveries. Photo: Sandbox Studio As work continues to complete the Large Hadron Collider in Europe and plans develop around the world for an International Linear Collider, one acceler- ator at the energy frontier is open for business right now. At Fermilab in Batavia, Illinois, the Tevatron collider is making discoveries. Michael Weber is working late this Tuesday night in mid- November, crunching data from his desk in a cubicle in Fermilab’s DZero building. He’s analyzing data collected by the DZero collider experiment. He is determined to wring every drop of information from the experiment’s vast and growing hoard of data. Just across the Tevatron ring, the scene is similar for Laura Sartori, working on the CDF experi- ment. Michael and Laura are looking for discoveries that could change particle physics forever. And the clock is ticking. Michael and Laura are not alone—far from it. Almost 1400 sci- entists, members of the CDF and DZero collaborations, are pouring on the effort to make the most of the US accelerator’s final run before CERN’s Large Hadron Collider takes over the energy frontier later in the decade. Long after normal working hours, the lights burn in the cubicles of the CDF and DZero offices as experimenters search for the tell-tale tracks that might lead them toward a sighting of supersymmetry, extra dimensions, dark matter, exotic particles, and a host of other phenomena that no one on the planet has ever seen before.
    [Show full text]
  • Research Resumé — Prof. Terry Wyatt
    Research Resum´e— Prof. Terry Wyatt FRS The Standard Model (SM) of particle physics describes the interactions of the gauge bosons (γ, Z, W±, gluons) with one another and with the fundamental fermions (the quarks and leptons). Over the past thirty years I have made a number of influential measurements at electron-positron and hadron- hadron colliders that have helped establish the SM as the precise theory of the elementary particles. My work has enabled significant improvements in the experimental precision with which: (a) the SM has been tested and (b) models of the possible new physics beyond the SM (BSM) have been constrained. In order to make these measurements I have developed a number of innovative techniques that have continued to find wide application within the field. In recognition of my contributions to hadron collider physics I was awarded the 2011 Chadwick medal and prize by the Institute of Physics. I was elected as a Fellow of the Royal Society (FRS) in 2013. My D.Phil. research was performed with the TASSO experiment at what was then the world’s highest energy e+e− collider, PETRA at DESY. This was before the discovery of the W and Z bosons and I chose to work on testing a very important prediction of the SM, namely that fermion-antifermion pairs should be produced with a forward-backward charge asymmetry in e+e− annihilation (arising from Z/γ interference). I made the first observation of this asymmetry in the bb final state. In order to make this measurement I developed the first successful algorithm to use kinematic information to distinguish b quark jets from the jets produced by other, lighter, quarks.
    [Show full text]
  • ELECTROWEAK MEASUREMENTS from RUN II at the TEVATRON TR WYATT Department of Physics and Astronomy, University of Manchester
    ELECTROWEAK MEASUREMENTS FROM RUN II AT THE TEVATRON T. R. WYATT Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK Email: [email protected] The CDF and DÂ detectors were fully commissioned for physics running in Run II at the Tevatron pp¹ collider in early 2002. Since then both experiments have collected data samples corresponding to an integrated luminosity of around L = 200 pb¡1 at a pp¹ centre-of-mass energy of ps = 1.96 TeV. Datasets corresponding L = 120 pb¡1 have beenR analyzed for physics so far. Recent electroweak measurements from Run II are reviewed.R Cross section times branching ratio measurements (σ Br) are presented for the intermediate vector bosons (IVB's) in their leptonic ¢ decay modes: W `º and Z `+`¡. For the ¯rst time, a combination of the σ Br results from the CDF and DÂ ! ! ¢ experiments is made; this includes using a consistent choice of the total inelastic pp cross section for the luminosity determinations of the two experiments. Quantities derived from these σ Br values are also updated. These include: ¢ R the ratio of the σ Br values for W and Z; Br(W `º), the leptonic branching ratio of the W ; and ¡W, the total ` ¢ ! decay width of the W . Other measurements using events containing W and Z leptonic decays are presented, including studies that probe the QCD phenomenology of W /Z production and searches for events containing two intermediate vector bosons. 1. Experimental Measurements of σ ¢ Br for Z ! `+`¡ and W ! `º 1.1. Introduction Figure 1 shows the mechanism for IVB production in pp¹ collisions.
    [Show full text]
  • Belief and Observation: the Top Quark and Other Tales of “Discovery”
    Belief and Observation: The Top Quark and Other Tales of “Discovery” T. Ferbel Universities of Rochester and Maryland “Seek, and Ye Shall Find” (Matthew 7:7) (If you search long enough, you’re bound to find something!) 1 Plan for the evening: • Story of the discovery of the top quark (1995) • Story of the stillbirth of the b* meson (1964) • Tragedy of the “splitting” of the A2 meson (≈1970) • A tale from “Pathological Science” (Langmuir ≈1930) • A few words on medical research!!! • Skip many other quirks: cold fusion, gravity waves, βν>1, N-rays, leptoquarks at DESY, “OopsLeon,“ etc, etc, from work of top scientists over past 100 years! • A word on human frailty (but hope) --------------------------- References: I. Langmuir, A. Wróblewski, S. Stone, others on web. 2 History of the top quark 1973: Makoto Kobayashi and Toshihide Maskawa predict the existence of a third generation of quarks in their attempt to accommodate the observed violation of CP invariance in K0 decays. (Cabibbo/GIM mixing combine in CKM!) 1974: The November revolution with discovery of the J/ψ and the fourth (GIM) “charm” quark at both BNL and SLAC by Sam Ting et al and Burt Richter et al, respectively, and, shortly thereafter, the τ lepton by Martin Perl et al (also at SLAC), with the τ providing major support for a third generation of fermions. 1975: Haim Harari, a great wizard (Israeli theorist) of the era, names the quarks of the third generation "top" and "bottom" to match the "up" and "down" quarks of the first generation, reflecting their "spin up" and "spin down" membership in a new weak-isospin doublet that also restores the numerical quark/lepton symmetry of the next (current) version of the standard model.
    [Show full text]
  • Arxiv:1312.4884V1 [Physics.Soc-Ph] 17 Dec 2013 Snowmass 2013 Electronic Proceedings Community Summer Study, Minneapolis, MN July 29 – August 6, 20123 Contents
    SLAC{PUB{15859 December, 2013 Benefits to the U.S. from Physicists Working at Accelerators Overseas Jacob Anderson, Raymond Brock, Yuri Gershtein, Nicholas Hadley, Michael Harrison, Meenakshi Narain, Jason Nielsen, Fred Olness, Bjoern Penning, Michael Peskin, Eric Prebys, Marc Ross, Salvatore Rappoccio, Abraham Seiden, Ryszard Stroynowski ABSTRACT We illustrate benefits to the U.S. economy and technological infrastructure of U.S. participation in accelerators overseas. We discuss contributions to exper- imental hardware and analysis and to accelerator technology and components, and benefits stemming from the involvement of U.S. students and postdoctoral fellows in global scientific collaborations. CONTRIBUTED TO arXiv:1312.4884v1 [physics.soc-ph] 17 Dec 2013 Snowmass 2013 Electronic Proceedings Community Summer Study, Minneapolis, MN July 29 { August 6, 20123 Contents 1 Introduction 2 2 U.S. Leadership in Fundamental Science 3 2.1 Today's Big Science Scale . 3 2.2 Sharing of effort in large science projects . 5 2.3 Sharing international responsibility for large projects . 7 3 Particle Physics Innovation-Transfer 7 3.1 Contributions to Detectors . 8 3.1.1 CMS endcap . 9 3.1.2 ATLAS pixel tracker . 9 3.2 Contributions to Accelerators . 11 3.2.1 Accelerator collaboration in overseas projects . 11 3.2.2 The LHC luminosity upgrade . 13 3.2.3 The ILC R&D program . 14 3.2.4 Accelerator innovation: conclusions . 15 4 Particle Physics Imagination-Transfer 16 4.1 Contributions to Experimental Analysis . 16 4.1.1 An analysis contributor { 1 . 16 4.1.2 An analysis contributor { 2 . 17 4.1.3 An analysis leader .
    [Show full text]
  • Evaluation of the Benefits That the UK Has Derived from CERN
    Evaluation of the benefits that the UK has derived from CERN Evidence Document August 2020 Evaluation of the benefits that the UK has derived from CERN Evidence Document technopolis |group| July 2020 Neil Brown Paul Simmonds Cristina Rosemberg Maike Rentel Charlotte Glass Antonella De Santo Table of Contents 1 Introduction .............................................................................................................................................. 1 2 Study scope and objectives ....................................................................................................................... 2 3 Approach and methods ............................................................................................................................ 2 4 CERN, its facilities and activities ............................................................................................................. 4 4.1 History and governance ........................................................................................................................ 4 4.2 Facilities and capabilities ...................................................................................................................... 5 4.3 Technology development ...................................................................................................................... 9 4.4 Contracts and procurement .................................................................................................................11 4.5 Knowledge transfer .............................................................................................................................
    [Show full text]
  • High Energy Colliders and the Rise of the Standard
    INSIGHT REVIEW NATURE|Vol 448|19 July 2007|doi:10.1038/nature06075 High-energy colliders and the rise of the standard model Terry Wyatt1 Over the past quarter of a century, experiments at high-energy particle colliders have established the standard model as the precise theory of particle interactions up to the 100 GeV scale. A series of important experimental discoveries and measurements have filled in most of the missing pieces and tested the predictions of the standard model with great precision. The standard model of particle physics describes the Universe as being strong interaction are the analogue of charge; antiquarks carry the composed of a rather small number of different types of elementary equivalent anticolour. A particular feature of the strong interaction is particle (see page 270) that interact in a small number of well-defined that coloured quarks cannot exist as free particles for more than about different ways. 10−24 s. The particles we observe in our detectors are hadrons — col- Interactions among the elementary particles are represented by Feyn- lections of quarks and/or antiquarks that have no net colour. There are man diagrams such as those in Fig. 1a. These show the annihilation of two basic types of hadron: mesons contain a quark and an antiquark (of an electron–positron (e+e−) pair to produce a fermion–antifermion pair opposite colour); baryons contain three quarks (one of each colour). (such as a quark–antiquark or lepton–antilepton pair), and such interac- When a high-energy quark or gluon is produced, it is observed as a tions are examples of the ‘electroweak’ interaction, which is propagated collimated ‘jet’ of hadrons.
    [Show full text]
  • Overview of Terry's 2019
    Overview of Terry’s 2019 Terry Wyatt. Manchester Christmas Meeting, 2019. Current PhD students • Sam Dysch: search for τ-lepton universality violation in W decays – Target precision ~1.5% for Run 2 data set (c.f. LEP-combined: 6.5%) • Diego Barón: τ-lepton identification at high pT • Lewis Higgins: Football (co-supervised with Tobias Galla) – EPSRC CASE – co-funded with Man.City) • Plus MPhys students (fysics and phootball) • Plus 10 fb-1 of 13 TeV ATLAS data in the 3rd year UG teaching lab. – First evidence for Higgs to 4-leptons in the 3rd year lab.! 2 Football • Data available: every game in 2016, 2017, 2018 and current premier league seasons • Technical work on datasets (in close collaboration with City expert) • Store in a consistent fashion data from different sources: position of players and ball, ball possession, game events • Now in a position to repeat/combine/extend studies previously performed as part of MPhys/summer projects Figure 7.14: Premier League 2017 - Optimised tiles on a per match basis. Velocity distorted, nearest player. Spatial Control: Voronoi regions boosted by player Correlation between “expected velocity and including consideration goals” and ”spatial control” of contested space 3 Figure 7.11: Diagram of the pixels created by the distorted Voronoi definition combined with the contested pixels (nearest home, nearest away) model. The distortedFigure Voronoi 7.15: model Premiercan be used League to modify 2018the standard - Optimised definition of tiles the Voronoi on a (nearest per match basis. Velocity distorted, nearest player. player by time, rather than distance) - figure 7.10 is an example of this.
    [Show full text]
  • 5Th International Masterclasses „Hands on Particle Physics“
    EPPOG International Masterclasses “Hands on Particle Physics“ www.physicsmasterclasses.org Plenary ECFA meeting, CERN, 26.11.2009 Michael Kobel, TU Dresden The masterclass idea Basic idea from UK Students (16-19 year-olds) spend 1 day at research institute Listen to scientists‘ introduction to particle physics Work like real scientists: measurements with particle physics data Why Masterclasses? Make modern particle physics data available to students Let students explore fundamental forces and building blocks of nature Demonstrate the scientific research process Stimulate interest in science The EPPOG international masterclass idea Create an international collaboration of students Join institutes worldwide with 300-400 students per day Since 2005: all w/in 3 weeks each year Over 80 institutes from 23 countries taking part Over 6000 students participating 5-6 masterclasses join in video conference at the end of the day Discuss results and differences Combine results (better accuracy) Quiz and prizes Questions to scientists schedule, data, background material, description of all participating institutes: www.physicsmasterclasses.org Participation EPPOG international masterclasses 25 120 20 100 80 15 60 10 40 5 20 0 0 2005 2006 2007 2008 2009 2005 2006 2007 2008 2009 Countries Institutes US 6000 (Quarknet) 5000 4000 3000 2000 1000 Brazil 0 2005 2006 2007 2008 2009 South Africa Participants Examples: Italy, Germany Hamburg Berlin Göttingen WuppertalDortmund Dresden Aachen Siegen Bonn Würzburg Mainz Erlangen Heidelberg Tübingen München Freiburg 2009: 14 institutes 2010: +2 institutes Agenda of the day Lectures Standard model, Accelerators, Detectors institute´s activities, cosmology etc. Lunch with physics students and tutors Measurements Video conference Lectures Measurements Collecting results Local analysis Final video conference: combination of results Quiz with the CERN moderators Prizes funded by CERN Masterclass CD-rom 10 web-based systems with material in 17 languages online at http://www.physicsmasterclasses.org physics offline on masterclass CDrom (ca.
    [Show full text]
  • Membership of Sectional Committees 2015
    Membership of Sectional Committees 2015 The main responsibility of the Sectional Committees is to select a short list of candidates for consideration by Council for election to the Fellowship. The Committees meet twice a year, in January and March. SECTIONAL COMMITTEE 1 [1963] SECTIONAL COMMITTEE 3 [1963] Mathematics Chemistry Chair: Professor Keith Ball Chair: Professor Anthony Stace Members: Members: Professor Philip Candelas Professor Varinder Aggarwal Professor Ben Green Professor Harry Anderson Professor John Hinch Professor Steven Armes Professor Christopher Hull Professor Paul Attfield Professor Richard Kerswell Professor Shankar Balasubramanian Professor Chandrashekhar Khare Professor Philip Bartlett Professor Steffen Lauritzen Professor Geoffrey Cloke Professor David MacKay Professor Peter Edwards Professor Robert MacKay Professor Malcolm Levitt Professor James McKernan Professor John Maier Professor Michael Paterson Professor Stephen Mann Professor Mary Rees Professor David Manolopoulos Professor John Toland Professor Paul O’Brien Professor Srinivasa Varadhan Professor David Parker Professor Alex Wilkie Professor Stephen Withers SECTIONAL COMMITTEE 2 [1963] SECTIONAL COMMITTEE 4 [1990] Astronomy and physics Engineering Chair: Professor Simon White Chair: Professor Hywel Thomas Members: Members: Professor Girish Agarwal Professor Ross Anderson Professor Michael Coey Professor Alan Bundy Professor Jack Connor Professor Michael Burdekin Professor Laurence Eaves Professor Russell Cowburn Professor Nigel Glover Professor John Crowcroft
    [Show full text]
  • Springer Theses
    Springer Theses Recognizing Outstanding Ph.D. Research For further volumes: http://www.springer.com/series/8790 Aims and Scope The series ‘‘Springer Theses’’ brings together a selection of the very best Ph.D. theses from around the world and across the physical sciences. Nominated and endorsed by two recognized specialists, each published volume has been selected for its scientific excellence and the high impact of its contents for the pertinent field of research. For greater accessibility to non-specialists, the published versions include an extended introduction, as well as a foreword by the student’s supervisor explaining the special relevance of the work for the field. As a whole, the series will provide a valuable resource both for newcomers to the research fields described, and for other scientists seeking detailed background information on special questions. Finally, it provides an accredited documentation of the valuable contributions made by today’s younger generation of scientists. Theses are accepted into the series by invited nomination only and must fulfill all of the following criteria • They must be written in good English. • The topic should fall within the confines of Chemistry, Physics, Earth Sciences, Engineering and related interdisciplinary fields such as Materials, Nanoscience, Chemical Engineering, Complex Systems and Biophysics. • The work reported in the thesis must represent a significant scientific advance. • If the thesis includes previously published material, permission to reproduce this must be gained from the respective copyright holder. • They must have been examined and passed during the 12 months prior to nomination. • Each thesis should include a foreword by the supervisor outlining the signifi- cance of its content.
    [Show full text]